高压下硅酸盐、金属和块状土熔体中氮掺入的比较研究

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Bijaya B Karki , Colin Jackson , Ekanshu Mallick , Abin Shakya , Dipta B Ghosh , Gabriele Morra
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引用次数: 0

摘要

氮作为大气中主要的挥发性元素,预计也存在于地球表面之下。它的内部预算和分布可能在很大程度上是由地核形成和其他过程决定的,这些过程导致了地球上挥发性物质的明显耗竭。为了更好地理解氮在原始地球经历多期岩浆海洋环境时的吸积阶段的表现,我们报告了在0至125 GPa(3000至5000 K)宽压力范围内硅酸盐熔体中氮的结合的第一性原理计算研究,以及在特定条件下富铁金属熔体和大块类地熔体中的氮。结果表明,在低压条件下,硅酸盐熔体中氮的形态几乎完全由N2分子组成,并有空隙占用。随着压力的增加,氮与硅酸盐网络的相互作用越来越大,与铁的结合比与熔体中存在的任何其他阳离子(Mg、Si、Ca、Al和Ni)的结合更强。压力和还原条件都有助于氮以氮化物形式化学溶解,从而促进地幔中可能存在的深层致密硅酸盐熔体的氮保留。金属液体通过与铁结合来吸收氮,与自身或其他杂质的相互作用很弱或没有相互作用。模拟的块状土熔体体系表现出相偏析,形成由硅酸盐区包围的富铁团簇。利用来自两相体系的相关局部配位统计量评估的氮的金属-硅酸盐分配系数在30.5 GPa (3000 K, IW-3.1)时为~ 31,在37.1 GPa (4000 K, IW-2.2)时为~ 18,在131 GPa (5000 K, IW-2.1)时为~ 24,与测量趋势基本一致。基于预测的对金属液体的强优先分配,我们认为,虽然氮可能从硅酸盐地幔中耗尽,但它可能被隔离在地核中。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A comparative study of nitrogen incorporation in silicate, metallic, and bulk earth melts at high pressure
Nitrogen as the dominant volatile element of the atmosphere is also expected to exist underneath the Earth’s surface. Its interior budget and distribution may have largely been set early on by the core formation and other processes that led to apparent volatile depletion in the terrestrial planet. To better understand how nitrogen may have behaved during the accretion stages when proto-Earth experienced multiple episodes of magma ocean environments, we report a first-principles computational study of nitrogen incorporation in silicate melts over wide pressure range 0 to 125 GPa (3000 to 5000 K), as well as in iron-rich metallic melt and bulk Earth-like melt at selected conditions. The results show that the speciation of nitrogen in silicate melts at low pressures consists of almost entirely N2 molecules with interstitial occupancy. As pressure increases, nitrogen interacts increasingly with the silicate network and bonds with iron more strongly than with any other cations (Mg, Si, Ca, Al, and Ni) present in the melt. Both pressure and reducing conditions help nitrogen chemically dissolve as nitride species thus promoting nitrogen retention of possible deep-seated dense silicate melts in the mantle. Metallic liquid incorporates nitrogen by bonding with iron with weak or no interactions with itself or with other impurities. The simulated bulk Earth melt system shows a phase segregation to form an iron-rich cluster which is surrounded by a silicate region. The metal-silicate partition coefficient of nitrogen evaluated using the relevant local coordination statistics from the two-phase system is ∼31 at 30.5 GPa (3000 K, IW-3.1), ∼18 at 37.1 GPa (4000 K, IW-2.2), and ∼24 at 131 GPa (5000 K, IW-2.1) which are generally consistent with the measured trends. Based on the predicted strong preferential partitioning to the metallic liquid, we argue that while nitrogen may be depleted from the silicate mantle, it may be sequestered in the core.
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来源期刊
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
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